Published April 1976 | Version v1
Report Metadata-only

Numerical models of astrophysical convection

Creators

  • 1. Cambridge Univ. (UK). Dept. of Applied Mathematics and Theoretical Physics

Description

Using the conservation laws for mass, linear momentum and energy the heat-transport is calculated within a simple star-model. (WL)

Abstract (German)

Aus den Erhaltungssaetzen fuer die Masse, den Impuls und die Energie wird fuer ein einfaches Sternmodell der Waermetransport numerisch berechnet. (WL)

Additional details

Publishing Information

Imprint Title
Computing in plasma physics and astrophysics. Proceedings
Imprint Pagination
vp.
Report number
IPP--6/147

Conference

Title
2. European conference on computational physics.
Dates
27 Apr 1976.
Place
Garching/Muenchen, Germany, F.R.

INIS

Country of Publication
Germany
Country of Input or Organization
Germany
INIS RN
8314330
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
CONVECTION; NONLINEAR PROBLEMS; NUMERICAL SOLUTION; STAR MODELS; STARS
Descriptors DEC
ENERGY TRANSFER; HEAT TRANSFER; MATHEMATICAL MODELS

Optional Information

Notes
1 fig.; with refs.
Secondary number(s)
AED-Conf--76-237-031.